\begin{document}$10^{-18}$\end{document}–\begin{document}$10^{-8}\;\mathrm{eV}$\end{document}. We present projected constraints for two candidate Mössbauer isotopes, \begin{document}$^{109}\mathrm{Ag}$\end{document} and \begin{document}$^{45}\mathrm{Sc}$\end{document}, with \begin{document}$^{109}\mathrm{Ag}$\end{document} providing the strongest sensitivity. For \begin{document}$^{109}\mathrm{Ag}$\end{document}, projected sensitivities of approximately \begin{document}$10^{-19}$\end{document}, \begin{document}$10^{-22}$\end{document}, and \begin{document}$10^{-21}\; \mathrm{GeV^{-1}}$\end{document} can be achieved for the scalar DM–photon, DM–gluon, and DM–quark couplings \begin{document}$f_{\gamma}^{-1}$\end{document}, \begin{document}$f_{g}^{-1}$\end{document}, and \begin{document}$f_{\hat{m}}^{-1}$\end{document}, respectively. In the low-mass region, the projected sensitivity to the scalar DM–photon coupling approaches current constraints from equivalence-principle (EP) tests. These results demonstrate that Mössbauer-based techniques provide a promising and competitive approach to probing ultralight dark matter interactions with Standard Model particles."> Searching for ultralight dark matter with Mössbauer resonance -
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